Kepler-141 is 982 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,910 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-141 b goes round its star every 3.11 days, 28 times as often as Mercury goes round the Sun.
| Surface temperature | 4,910 K |
| Mass | 0.878 solar masses |
| Radius | 0.787 solar radii |
| Luminosity | 0.3579 times the Sun |
| Apparent magnitude | 13.624 |
| Age | about 12.39 billion years |
| Distance from the Sun | 982.3 light-years (301.2 parsecs) |
| Position (J2000) | RA 297.9707°, Dec 47.7316° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-141 b | 3.11 days | 0.0390 AU | 0.69 R⊕ | 0.257 M⊕ estimated | Transit, 2014 |
| Kepler-141 c | 7.01 days | 0.0670 AU | 1.41 R⊕ | 2.57 M⊕ estimated | Transit, 2014 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.
For a star of 4,910 K, 0.36 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.60 to 1.08 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 982 years ago, around 1040.